We are utilizing a combination of nuclear reaction rate measurements, computational modelling, and presolar grain isotopic measurements to test the viability of the neutrino-driven wind in a core collapse supernova as a source of elements between selenium and silver. If successful, we will resolve open questions about the weak rapid neutron capture process, thereby making a significant contribution to the field of nuclear astrophysics.
Ong, W. 2019. "Nuclear Astrophysics Research with the MUSIC Detector." Nuclear Physics Opportunities at ATLAS, ANL, July 2019. LLNL-PRES-781259.
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